Black hole boundaries

By I. Booth. 2005

307 citations recorded by the source corpus.

Classical black holes and event horizons are highly nonlocal objects, defined in relation to the causal past of future null infinity. Alternative, quasilocal characterizations of black holes are often used in mathematical, quantum, and numerical relativity. These include apparent, Killing, trapping, isolated, dynamical, and slowly evolving horizons. All of these are closely associated with two-surfaces of zero outward null expansion. This paper reviews the traditional definition of black holes and provides an overview of some of the more recent work on alternative horizons.PACS Nos.: 04.20.Cv, 04.70.–s, 04.70.Bw

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics, Statistical and Nonlinear Physics

View Paper: https://www.semanticscholar.org/paper/9d47988e5fff9ef6a781fac0ae40d49effcb7fab

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In Astronomy and Astrophysics

  1. M. Rangamani
  2. V. Hubeny
  3. Sayantani Bhattacharyya
  4. Shiraz Minwalla
  5. R. Loganayagam
  6. Harvey Reall
  7. Esperanza Lopez
  8. Gautam Mandal

In Nuclear and High Energy Physics

  1. M. Rangamani
  2. V. Hubeny
  3. Shiraz Minwalla
  4. Sayantani Bhattacharyya
  5. T. Takayanagi
  6. R. Loganayagam
  7. A. Allais
  8. Esperanza Lopez

In Statistical and Nonlinear Physics

  1. M. Rangamani
  2. V. Hubeny
  3. Shiraz Minwalla
  4. E. Tonni
  5. A. Allais
  6. Sayantani Bhattacharyya
  7. Harvey Reall
  8. T. Takayanagi

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